Age is one of the most fundamental parameters of a star, yet it is one of the hardest to
determine as it requires modelling various aspects of stellar formation and evolution. When …

Most stars form in highly clustered environments within molecular clouds, but eventually
disperse into the distributed stellar field population. Exactly how the stellar distribution …

We perform simulations of star cluster formation to investigate the morphological evolution of
embedded star clusters in the earliest stages of their evolution. We conduct our simulations …

Star clusters are among the first celestial objects catalogued by early astronomers. As
simple and coeval populations, their study has been instrumental in charting the properties …

Molecular hydrogen clouds are a key component of the interstellar medium because they
are the birthplaces for stars. They are embedded in atomic gas that pervades the interstellar …

It remains unclear how galactic environment affects star formation and stellar cluster
properties. This is difficult to address in Milky Way-mass galaxy simulations because of …

Observations of clusters suffer from issues such as completeness, projection effects,
resolving individual stars, and extinction. As such, how accurate measurements and …

We analyze the far-ultraviolet (1130− 1770 Å rest frame) spectroscopy of 20 young (< 50
Myr) and massive (> 10 4 M⊙) star clusters (YSCs) in 11 nearby star-forming galaxies. We …

We use the largest catalog of open clusters in the post-Gaia era to provide an observational
view of the Galactic disk. By compiling physical parameters such as age, distance, and …

We have studied the kinematics of a unique sample of young open star clusters (OSCs) with
high vertical velocities, km s. The characteristics of these clusters were taken from the …